Thermodynamics and Transport Properties of the CeBr3 - MBr Binary Systems

2019 ◽  
Vol 3 (35) ◽  
pp. 453-465
Author(s):  
Marcelle Gaune-Escard ◽  
Leszek Rycerz ◽  
Ewa Ingier-Stocka ◽  
Slobodan Gadzuric
Keyword(s):  
Transport Properties ◽  
Binary Systems

Combined NMR and molecular dynamics modeling study of transport properties in sulfonamide based deep eutectic lithium electrolytes: LiTFSI based binary systems

2016 ◽  
Vol 18 (9) ◽  
pp. 6657-6667 ◽  
Author(s):  
Allen D. Pauric ◽  
Ion C. Halalay ◽  
Gillian R. Goward
Keyword(s):  
Molecular Dynamics ◽  
Transport Properties ◽  
Binary Systems ◽  
Electrolyte Solutions ◽  
Electrochemical Stability ◽  
Li Ion Batteries ◽  
Dynamics Modeling ◽  
Molecular Dynamics Modeling ◽  
Li Ion ◽  
Modeling Study

The trend toward Li-ion batteries operating at increased (>4.3 V vs. Li/Li+) voltages requires the development of novel classes of lithium electrolytes with electrochemical stability windows exceeding those of LiPF6/carbonate electrolyte solutions.

Thermodynamic and transport properties of the PrBr3–MBr binary systems (M=Li, Na)

2009 ◽  
Vol 148 (1) ◽  
pp. 40-44 ◽  
Author(s):  
Ewa Ingier-Stocka ◽  
Leszek Rycerz ◽  
Madjid Berkani ◽  
Marcelle Gaune-Escard
Keyword(s):  
Transport Properties ◽  
Binary Systems ◽  
Thermodynamic And Transport Properties

Some Results of the Spectroscopic Study of Four Close Binary Systems of Early Spectral Types

1965 ◽  
Vol 5 ◽  
pp. 120-130
Author(s):  
T. S. Galkina
Keyword(s):  
Spectroscopic Study ◽  
Spectral Type ◽  
Spectroscopic Investigation ◽  
Binary Systems ◽  
Quantitative Information ◽  
Close Binary ◽  
Physical Parameters ◽  
Absorption And Emission ◽  
Close Binary Systems ◽  
Quantitative Estimates

It is necessary to have quantitative estimates of the intensity of lines (both absorption and emission) to obtain the physical parameters of the atmosphere of components.Some years ago at the Crimean observatory we began the spectroscopic investigation of close binary systems of the early spectral type with components WR, Of, O, B to try and obtain more quantitative information from the study of the spectra of the components.

Quasi-Periodic Oscillations in Dwarf Novae

1979 ◽  
Vol 46 ◽  
pp. 77-88
Author(s):  
Edward L. Robinson
Keyword(s):  
Binary Systems ◽  
Outer Edge ◽  
Light Curves ◽  
Close Binary ◽  
Bright Spot ◽  
Dwarf Novae ◽  
Periodic Oscillations ◽  
High Frequencies ◽  
Short Period ◽  
Typical Time

Three distinct kinds of rapid variations have been detected in the light curves of dwarf novae: rapid flickering, short period coherent oscillations, and quasi-periodic oscillations. The rapid flickering is seen in the light curves of most, if not all, dwarf novae, and is especially apparent during minimum light between eruptions. The flickering has a typical time scale of a few minutes or less and a typical amplitude of about .1 mag. The flickering is completely random and unpredictable; the power spectrum of flickering shows only a slow decrease from low to high frequencies. The observations of U Gem by Warner and Nather (1971) showed conclusively that most of the flickering is produced by variations in the luminosity of the bright spot near the outer edge of the accretion disk around the white dwarf in these close binary systems.

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